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Some Observable Physical Properties of the Higher Dimensional dS/AdS Black Holes in Einstein-Bumblebee Gravity Theory

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arxiv 2207.10122 v3 pith:73CUCDAI submitted 2022-07-20 hep-th gr-qc

Akhil Uniyal , Sara Kanzi , İzzet Sakall{i} This is my paper · ORCID
classification hep-thgr-qc
keywords blackdimensionalhigherholede-sittereinstein-bumblebeefactorsgravity
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We study the greybody factors, quasinormal modes, and shadow of the higher dimensional de-Sitter (dS)/ anti de-Sitter (AdS) black hole spacetimes derived from the Einstein-bumblebee gravity theory within the Lorentz symmetry breaking (LSB) framework. We specifically apply the semi-analytical WKB method and the time domain approach to study the scalar and Dirac perturbations of the black hole. In-depth researches are done on the effects of the LSB and dimensionality on the bosonic/fermionic greybody factors, quasinormal modes, and shadow of the higher dimensional bumblebee black hole. The results obtained are discussed, tabulated, and illustrated graphically.

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Cited by 2 Pith papers

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  1. Perturbative black-hole and horizon solutions in gravity with explicit spacetime-symmetry breaking

    gr-qc 2024-11 conditional novelty 6.0 of 10

    New perturbative black hole solutions in an explicit spacetime-symmetry-breaking gravity EFT, with derived observables including three-horizon metrics when two coefficients are active.

  2. Exact Black Hole Solutions in Bumblebee Gravity with Lightlike or Spacelike VEVS

    gr-qc 2025-10 conditional novelty 5.0 of 10

    New exact Schwarzschild-like, (A)dS-like, and charged black holes in bumblebee gravity with a two-component vector VEV keep Lorentz-violating corrections even when the VEV is lightlike, with Wald and first-law entropi...

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